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相关论文: Slow-roll inflation in Palatini $F(R)$ gravity

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It is generally believed that in single-field slow-roll inflation, a large tensor-to-scalar ratio $r > 0.1$ requires inflaton field values close to or above the Planck scale. Recently, it has been claimed that $r > 0.15$ can be achieved…

高能物理 - 唯象学 · 物理学 2014-05-29 Stefan Antusch , David Nolde

In this work we shall study a class of $f(R,\phi)$ gravity models which during the inflationary era, which is the large curvature regime, result to an effective inflationary Lagrangian that contains a rescaled Einstein-Hilbert term $\alpha…

广义相对论与量子宇宙学 · 物理学 2022-03-14 V. K. Oikonomou , Ifigeneia Giannakoudi , Achilles Gitsis , Konstantinos-Rafail Revis

In previous work, two of us have proposed a model of inflationary magnetogenesis based on a rolling auxiliary field able both to account for the magnetic fields inferred by the (non) observation of gamma-rays from blazars, and to start the…

宇宙学与河外天体物理 · 物理学 2018-06-13 Chiara Caprini , Maria Chiara Guzzetti , Lorenzo Sorbo

We study a model of inflation with terms quadratic and logarithmic in the Ricci scalar, where the gravitational action is $f(R)=R+\alpha R^2+\beta R^2 \ln R$. These terms are expected to arise from one loop corrections involving matter…

高能物理 - 理论 · 物理学 2015-06-19 Ido Ben-Dayan , Shenglin Jing , Mahdi Torabian , Alexander Westphal , Lucila Zarate

Inflationary slow-roll dynamics in Einstein gravity with a non-minimal scalar-curvature coupling can be equivalent to that in the certain f(R) gravity theory. We review the correspondence and extend it to N=1 supergravity. The non-minimal…

高能物理 - 理论 · 物理学 2015-06-04 Sergei V. Ketov , Alexei A. Starobinsky

We explore conformal-anomaly driven inflation in $F(R)$ gravity without invoking the scalar-tensor representation. We derive the stress-energy tensor of the quantum anomaly in the flat homogeneous and isotropic universe. We investigate a…

高能物理 - 理论 · 物理学 2014-08-13 Kazuharu Bamba , R. Myrzakulov , S. D. Odintsov , L. Sebastiani

A scalar potential obtained from the $D$-term in the Supergravity models, which dominates over $F$ term and is mainly responsible for the inflationary phase in the early universe, is studied. The potential with canonical kinetic terms for…

宇宙学与河外天体物理 · 物理学 2022-03-18 Rathin Adhikari , Mayukh R. Gangopadhyay , Yogesh

In this paper we study some classes of $\alpha$-attractors models in the Jordan frame and we find the corresponding $F(R)$ gravity theory. We study analytically the problem at leading order and we investigate whether the attractor picture…

广义相对论与量子宇宙学 · 物理学 2017-01-04 S. D. Odintsov , V. K. Oikonomou

f(R) gravity theories in the Palatini formalism has been recently used as an alternative way to explain the observed late-time cosmic acceleration with no need of invoking either dark energy or extra spatial dimension. However, its…

广义相对论与量子宇宙学 · 物理学 2012-12-07 Janilo Santos , Crislane de Souza Santos

This study examines how inflationary dynamics are affected by $f(R)$ theories with a non-minimal coupling between matter and curvature. Both positive and negative corrections to the minimal coupling of General Relativity are considered, and…

广义相对论与量子宇宙学 · 物理学 2026-01-29 Miguel Barroso Varela , Orfeu Bertolami , Andreas Mantziris

We consider inflation with a constant rate of rolling in which a complex scalar field plays the role of inflaton during the inflationary epoch. We implement the inflationary analysis for an accredited angular speed $\dot{\theta}$ which…

广义相对论与量子宇宙学 · 物理学 2024-05-16 Ramón Herrera , Mehdi Shokri , Jafar Sadeghi

In this paper, we demonstrate that a unified description of early and late-time acceleration is possible in the context of mimetic $F(R)$ gravity. We study the inflationary era in detail and demonstrate that it can be realized even in…

广义相对论与量子宇宙学 · 物理学 2016-12-21 S. Nojiri , S. D. Odintsov , V. K. Oikonomou

The inflation model with non-minimal coupling scalar field in the context of the hybrid metric Palatini is studied in this paper. We derive the Einstein's field equations, the equations of motion of the scalar field. Furthermore,the…

广义相对论与量子宇宙学 · 物理学 2024-02-29 Brahim Asfour , Aatifa Bargach , Ahmed Errahmani , Taoufik Ouali

The slow roll approximation is studied for cosmological models in Hyperextended Scalar-Tensor Theories of Gravity. A procedure to obtain slow roll solutions in non-minimally coupled gravity is outlined and some examples are provided. An…

广义相对论与量子宇宙学 · 物理学 2009-10-28 Diego F. Torres

We study Quadratic Inflation with the inflaton field $\phi$ coupled non-minimally to the curvature scalar $R$, so that the potential during inflation is of the form $V\propto m^2\phi^2+\xi R\phi^2$. We show that with a suitable choice of…

宇宙学与河外天体物理 · 物理学 2017-12-13 Tommi Tenkanen

We review the recent literature on modified theories of gravity in the Palatini approach. After discussing the motivations that lead to consider alternatives to Einstein's theory and to treat the metric and the connection as independent…

广义相对论与量子宇宙学 · 物理学 2011-05-09 Gonzalo J. Olmo

The $R^2$ inflation which is an extension of general relativity (GR) by quadratic scalar curvature introduces a quasi-de Sitter expansion of the early Universe governed by Ricci scalar being an eigenmode of d'Alembertian operator. In this…

高能物理 - 理论 · 物理学 2023-07-21 Alexey S. Koshelev , K. Sravan Kumar , Alexei A. Starobinsky

Although several models of $f(R)$ theories of gravity within the Palatini approach have been studied already, the interest was concentrated on those that have an effect on the late-time evolution of the universe, by the inclusion for…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Thomas P. Sotiriou

Recently, corrections to the standard Einstein-Hilbert action are proposed to explain the current cosmic acceleration in stead of introducing dark energy. We discuss the Palatini formulation of the modified gravity with a $\ln R$ term…

高能物理 - 理论 · 物理学 2009-11-10 Xin-He Meng , Peng Wang

In this work, we show that, in the presence of non-minimal coupling to gravity, it is possible to generate sizeable tensor modes in single-field models without transplanckian field values. These transplanckian field values apparently needed…

高能物理 - 唯象学 · 物理学 2015-07-14 G. Barenboim , O. Vives
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